2012
DOI: 10.1038/nature10827
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Magnetic reconnection from a multiscale instability cascade

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Cited by 75 publications
(111 citation statements)
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“…The RT instability quickly erodes and breaks the jet structure, leading to fast magnetic reconnection. 20,24 Hydrogen plasmas are found to develop kink instability in a very similar manner; but no distinct RT instability has been observed for hydrogen jets with g $ 10 10 m/s 2 ; RT instabilities with axial wavelength k z ¼ 3 À 5 cm are observed only in some rare shots with strong lateral acceleration g ¼ 10 11 À 3 Â 10 11 m/s 2 . We name the two cases as type I and type II hydrogen jets, respectively.…”
Section: Introductionmentioning
confidence: 90%
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“…The RT instability quickly erodes and breaks the jet structure, leading to fast magnetic reconnection. 20,24 Hydrogen plasmas are found to develop kink instability in a very similar manner; but no distinct RT instability has been observed for hydrogen jets with g $ 10 10 m/s 2 ; RT instabilities with axial wavelength k z ¼ 3 À 5 cm are observed only in some rare shots with strong lateral acceleration g ¼ 10 11 À 3 Â 10 11 m/s 2 . We name the two cases as type I and type II hydrogen jets, respectively.…”
Section: Introductionmentioning
confidence: 90%
“…3 of Ref. 20. This simple semi-quantitative analysis shows that the perturbation can be considered to be incompressible…”
Section: Perturbation and Linearizationmentioning
confidence: 99%
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“…The major features visible in the coded aperture image are the jet front and the kinking of the jet axis. 11,15,16,19,20 The relative intensities of the jet front and the jet axis differ by a factor of 20-50. The jet axis undergoes a kink instability where the axis accelerates into an expanding spiral.…”
Section: A Image Reconstructionmentioning
confidence: 99%
“…However, on observing electron and ion heating in a merging experiment, Ono et al 23 argued that electrons are Ohmically heated, whereas ions are heated by shock or viscous damping in the reconnection exhaust. 23 We report the following sequence of experimental observations of a spontaneous three-dimensional (3-D) Hallmediated reconnection: (i) a current-carrying MHD-driven plasma jet self-forms, 24 (ii) the jet undergoes a kink instability, 25 (iii) the kink provides the environment for development of a secondary, Rayleigh-Taylor (RT) instability, 26 (iv) the RT instability chokes the current channel radius to cause a fast localized reconnection, 26 (v) the reconnection produces localized electron and ion heating, and (vi) the reconnection also radiates broadband obliquely propagating, right-hand circularly polarized whistler waves. These observations show that Hall physics is important even though the plasma jet is collisional, that electrons are plausibly heated by Ohmic dissipation, and that ions are plausibly heated stochastically.…”
Section: Introductionmentioning
confidence: 99%